Cooling of a Compact Star with a LOFF Matter Core

Details Cooling of a Compact Star with a LOFF Matter Core Cooling of a Compact Star with a LOFF Matter Core

2006-10-30

arxiv.org/abs/hep-ph/0610404v1

Phys.Part.Nucl.39:1167-1169,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

3 pages, 1 figure, to appear in the proceedings of the Helmoltz International Summer School of Theoretical Physics on Dense Ma

Scientific paper

10.1134/S1063779608070332

Specific heat and neutrino emissivity due to direct URCA processes for quark
matter in the color superconductive Larkin-Ovchinnikov-Fulde-Ferrell (LOFF)
phase of Quantum-Chromodynamics have been evaluated. The cooling rate of
simplified models of compact stars with a LOFF matter core is estimated.

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